Prof. Dimitra Rigopoulou: Publications

A radio-jet driven outflow in the Seyfert 2 galaxy NGC 2110?

(2023)

Authors:

L Peralta de Arriba, A Alonso-Herrero, S García-Burillo, I García-Bernete, M Villar-Martín, B García-Lorenzo, R Davies, DJ Rosario, SF Hönig, NA Levenson, C Packham, C Ramos Almeida, M Pereira-Santaella, A Audibert, E Bellocchi, EKS Hicks, A Labiano, C Ricci, D Rigopoulou

Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3

(2023)

Authors:

Han Lei, Francesco Valentino, Georgios E Magdis, Vasily Kokorev, Daizhong Liu, Dimitra Rigopoulou, Shuowen Jin, Emanuele Daddi

A Diverse Population of z ~ 2 ULIRGs Revealed by JWST Imaging

(2023)

Authors:

J-S Huang, Zi-Jian Li, Cheng Cheng, Meicun Hou, Haojing Yan, SP Willner, Y-S Dai, XZ Zheng, J Pan, D Rigopoulou, T Wang, Zhiyuan Li, Piaoran Liang, A Esamdin, GG Fazio

A solar metallicity galaxy at z > 7? Possible detection of the [N ii] 122 μm and [O iii] 52 μm lines

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 521:2 (2023) 2526-2534

Authors:

Meghana Killi, Darach Watson, Seiji Fujimoto, Hollis Akins, Kirsten Knudsen, Johan Richard, Yuichi Harikane, Dimitra Rigopoulou, Francesca Rizzo, Michele Ginolfi, Gergö Popping, Vasily Kokorev

Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory

Space Science Reviews Springer 219:1 (2023) 9

Authors:

Susanne Aalto, Cara Battersby, Gordon Chin, Leslie K Hunt, Dimitra Rigopoulou, Antony A Stark, Serena Viti, Christopher K Walker

Abstract:

The Orbiting Astronomical Satellite for Investigating Stellar Systems (OASIS), a\ua0proposed Astrophysics MIDEX-class mission concept, has an innovative 14-meter diameter inflatable primary mirror that will provide the sensitivity to study far-infrared continuum and line emission from galaxies at all redshifts with high spectral resolution heterodyne receivers. OASIS will have the sensitivity to follow the water trail from galaxies to the comets that create oceans. It will bring an understanding of the role of water in galaxy evolution and its part of the oxygen budget, by measuring water emission from local to intermediate redshift galaxies, observations that have not been possible from the ground. Observation of the ground-state HD line will accurately measure gas mass in a wide variety of astrophysical objects. Thanks to its exquisite spatial resolution and sensitivity, OASIS will, during its one-year baseline mission, detect water in galaxies with unprecedented statistical significance. This paper reviews the extragalactic science achievable and planned with OASIS

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